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Dependence of ultraviolet (erythemal and total) radiation and CMF values on total and low cloud covers in Central Spain

机译:西班牙中部的紫外线(红斑和总辐射)和CMF值对总云量和低云量的依赖性

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摘要

The cloudiness effect on solar ultraviolet radiation (UV) has been analyzed in this study. Measurements of erythemal and UV total radiations have been registered in Valladolid, Central Spain (lat 41° 40'N, long. 4° 50'W and 840 m a.s.l.). A statistical analysis of cloudiness has been carried out resulting clear skies (0-2 oktas) the most frequent conditions under low cloud cover, while cloudy skies (6-7 oktas) are the prevailing under total cloud cover. Hence, the dependences of erythemal UV (UVER) and UV total (UVT) radiations and CMF values (on both ranges) on total and low cloud covers have been analyzed. In all cases, low clouds show higher attenuation than total cloud cover. Moreover, an empirical formula proposed by other authors for several Spanish cities is verified with very similar coefficients for Valladolid database. Finally, the dependence of the ratio between CMF values on UVER and UVT radiations on cloud cover and solar elevation angle is analyzed. As a result UVER and UVT radiations are not affected by the clouds in the same way. Actually, for low solar elevation angles, UVER is not as attenuated as UVT radiation. However, for high ones under cloudy (6-7 oktas) and, particularly, overcast (8 oktas) conditions, UVER presents smaller CMF values and, therefore, a higher attenuation. Due to the different spectral ranges between erythemal and UV total radiations, the photon reflections above the cloud, the Rayleigh scattering and the interaction of UV radiation with atmospheric components like ozone could explain these effects.
机译:在这项研究中分析了云量对太阳紫外线辐射的影响。在西班牙中部的巴利亚多利德已经记录了红斑和紫外线总辐射的测量值(北纬41°40',长4°50'W和840 m a.s.l.)。进行了多云度的统计分析,得出在低云量覆盖下最晴朗的天空(0-2 oktas)是最常见的情况,而在总云量覆盖下主要是多云天空(6-7 oktas)。因此,已经分析了红斑紫外线(UVER)和紫外线总量(UVT)辐射以及CMF值(在两个范围内)对总云量和低云量的依赖性。在所有情况下,低云的衰减都高于总云量。此外,用西班牙瓦拉多利德数据库的系数非常相似,验证了其他作者针对西班牙几个城市提出的经验公式。最后,分析了CMF值对云层覆盖的UVER和UVT辐射与太阳仰角之间的比率的依赖性。结果,UVER和UVT辐射不会以相同的方式受到云的影响。实际上,对于低太阳仰角,UVER的衰减不如UVT辐射大。但是,对于多云(6-7 oktas),尤其是阴天(8 oktas)条件下的高噪声,UVER的CMF值较小,因此衰减较高。由于红斑和紫外线总辐射之间的光谱范围不同,云层上方的光子反射,瑞利散射以及紫外线与大气成分(如臭氧)的相互作用可以解释这些影响。

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  • 来源
    《Atmospheric research》 |2010年第1期|p.21-27|共7页
  • 作者单位

    Atmosphere & Energy Lab, Applied Physics Department, Valladolid University, Prado de la Magdalena Street s, 47005, Valladolid, Spain;

    Atmosphere & Energy Lab, Applied Physics Department, Valladolid University, Prado de la Magdalena Street s, 47005, Valladolid, Spain;

    Atmosphere & Energy Lab, Applied Physics Department, Valladolid University, Prado de la Magdalena Street s, 47005, Valladolid, Spain;

    Atmosphere & Energy Lab, Applied Physics Department, Valladolid University, Prado de la Magdalena Street s, 47005, Valladolid, Spain;

  • 收录信息
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

    ultraviolet solar radiation; erythemal radiation; cloudiness; cloud modification factor;

    机译:紫外线太阳辐射;红斑辐射浑浊云修正因子;
  • 入库时间 2022-08-18 03:36:09

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